Biographical Encyclopedia of Astronomers

2014 Edition
| Editors: Thomas Hockey, Virginia Trimble, Thomas R. Williams, Katherine Bracher, Richard A. Jarrell, Jordan D. MarchéII, JoAnn Palmeri, Daniel W. E. Green

de Sitter, Willem

  • Adriaan Blaauw
Reference work entry
DOI: https://doi.org/10.1007/978-1-4419-9917-7_1284

Alternate Name

 Sitter, Willem de

BornSneek, the Netherlands, 6 May 1872

DiedLeiden, The Netherlands, 20 November 1934

Dutch mathematical astronomer Willem de Sitter gave his name to one of the first solutions to   Albert Einstein ’s equations of general relativity, which showed that a universe containing very little matter would, in some sense, expand, and so prepared the way for   Edwin Hubble ’s discovery of that expansion (though a different solution in fact applies). De Sitter was the son of a judge, Lamoraal U. de Sitter and Catharine Th. W. Bertling. He received his early education at Arnhem, the Netherlands, where his father was President of the Court. De Sitter studied at the University of Groningen, primarily in mathematics, under   Jacobus Kapteyn , with whom he maintained a lifelong friendship and scientific collaboration, receiving a Ph.D. in 1901 for work involving observations of the satellites of Jupiter, made in Cape Town, South Africa (1897–1899). In Cape Town, de Sitter also met and married Eleonore Suermondt. They had three sons and two daughters.

From his position as a staff member at Groningen, de Sitter was appointed to a professorship of astronomy at Leiden University in 1908, where he became director of the observatory in 1919, holding both positions until his death. He reorganized the Department of Astronomy at Leiden, adding a department for astrophysics, and observational facilities at the Union Observatory in Johannesburg, South Africa.

De Sitter has become best known for his work on cosmology, but the earliest part of his career and much of his later life were devoted to celestial mechanics and astrometry. In his thesis of 1901, he discussed heliometer observations of Jupiter’s inner moons made at the Cape Observatory, leading to an improved determination of the masses of these satellites. In a subsequent work (New Mathematical Theory of Jupiters Satellites), de Sitter presented a comprehensive analysis of the observations of the satellites made since 1668. His wide knowledge of celestial mechanics also allowed him to present comprehensive discussions of the complicated interrelations among the phenomena from which the major astronomical constants are derived, in particular the combination of results from geodetic and gravity measurements with those from astronomical observations. In 1927, he published The Most Probable Values of Some Astronomical Constants. A second paper On the System of Astronomical Constants, edited by de Sitter’s pupil  Dirk Brouwer, was posthumously published in 1938. These constants include both the shape of the Earth and numbers for the length of the astronomical unit and the masses of the planets.

In order to arrive at a system of fundamental declinations, free from the systematic errors due to atmospheric refraction and flexure of the telescope that always have plagued meridian observations, de Sitter initiated in 1930 a pilot expedition to Kenya, where, right on the Equator, declinations were made by measuring the distance along the horizon between the rising and setting points of a star, which gives an angle that is two times the complement of the declination.

De Sitter was among the very first to realize the importance of Einstein’s work on relativity for astronomy, and he contributed much to the introduction into the English-speaking countries of Einstein’s work during World War I. He first discussed, in 1911, the small deviations in the motions of the Moon and the planets still left in the context of classical dynamics. In 1916 and 1917, de Sitter presented to the Royal Astronomical Society a series of three papers on “Einstein’s Theory of Gravitation and its Astronomical Consequences.” Because there was almost no communication between Germany and England during World War I, these papers were instrumental in introducing general relativity to the English scientific community, and they played an important part in the decision made by   Arthur Eddington and others to send expeditions to observe the solar eclipse of 1919 to look for the small shifts in the positions of stars predicted by Einstein’s theory. In the context of his cosmological work, de Sitter introduced a solution to the fundamental equations that define the properties of the universe; it soon became known as the de Sitter universe (or de Sitter space), an alternative to Einstein’s solution, provided the density of matter in the universe could be considered negligible and the universe be allowed to expand. De Sitter’s solution predicted systematic redshifts in the spectra of distant objects (though a quadratic relationship rather than a linear one, which was sought by several colleagues).

De Sitter was elected president of the International Astronomical Union for 1925–1928. One of his major concerns (shared by Eddington and others) was to reintegrate the international community, and he succeeded in extending invitations to the 1928 General Assembly in Leiden to astronomers from Germany and others of the “Central Powers,” though some of these nations were not admitted to the union until after World War II. De Sitter was the author of a booklet on the history of the Leiden Observatory (1633–1933) and a founder (in 1921) of the journal Bulletin of the Astronomical Institutes of the Netherlands. It, in turn, was merged in 1969 with journals from France and Germany to form a single European journal, Astronomy and Astrophysics.

De Sitter received medals from the Royal Astronomical Society (London) and the Astronomical Society of the Pacific, as well as a number of honorary degrees.

The archives of Leiden Observatory have a collection of de Sitter’s notes and letters.

Selected References

  1. Blaauw, A. (1975). “Sitter, Willem de.” In Dictionary of Scientific Biography, edited by Charles Coulston Gillispie. Vol. 12, p. 448–450. New York: Charles Scribner’s Sons.Google Scholar
  2. De Sitter, W. (1925). “New Mathematical Theory of Jupiter’s Satellites.” Annals Leiden Observatory12: 1–83.Google Scholar
  3. De Sitter, W. (1931). “Jupiter’s Galilean Satellites.” Monthly Notices of the Royal Astronomical Society91: 706–738. (George Darwin Lecture, 8 May 1931.)ADSCrossRefGoogle Scholar
  4. — (1932). Kosmos: A Course of Six Lectures on the Development of Our Insight into the Structure of the Universe. Cambridge, Massachusetts: Harvard University Press. (A historical review of research on the structure of the Universe is in his monograph.)Google Scholar
  5. — (1933). The Astronomical Aspect of the Theory of Relativity. Berkeley: university of California Press. (Published shortly before his death.)Google Scholar
  6. Jones, H. Spencer (1935). “Willem de Sitter.” Monthly of the Notices Royal Astronomical Society95: 343–347.CrossRefGoogle Scholar
  7. Macpherson, H. (1933). Makers of Astronomy. Oxford: Clarendon Press, Chap. 8.MATHGoogle Scholar
  8. Oort, J. H. (1935). “Obituary”. Observatory58: 22–27.ADSGoogle Scholar
  9. Van der Kruit, P. C. and K. van Berkel (2000). The Legacy of Kapteyn; Studies on Kapteyn and the Development of Modern Astronomy. Dordrecht: Kluwer: Academic Publishers. (His grandson W. R. de Sitter contributed “Kapteyn and de Sitter; a Rare and Special Teacher-Student and Coach-Player Relationship,” pp. 79–108.)CrossRefGoogle Scholar

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© Springer Science+Business Media New York 2014

Authors and Affiliations

  • Adriaan Blaauw
    • 1
  1. 1.GroningenThe Netherlands